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VLBI Observations of SNR in M82 - Is 41.95+575 an Anomalous SNR or Something Else ?
Published online by Cambridge University Press: 13 May 2016
Abstract
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Global VLBI 1.7GHz datasets from 1990 and 1998 have been used to study the evolution of SNR 41.95+575 in M82. An expansion velocity of around 1800 km/s is found with an implied birth around 1915. A young 41.95+575 would resemble radio supernovae seen in Arp220, although it could also be an evolving accretion disc system
- Type
- Supernovae, Pulsars, and the Interstellar Medium
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2001
References
Kronberg, P.P., Sramek, R.A., Birk, G.T., Dufton, Q.W., Clarke, T.E., & Allen, M.L., 2000, ApJ, 535, 706.CrossRefGoogle Scholar
Pedlar, A., Muxlow, T.W.B., Garrett, M.A., Diamond, P.J., Wills, K.A., Wilkinson, P.N., & Alef, W., 1999, MNRAS, 307, 761.CrossRefGoogle Scholar
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